JINA - Virtual Journal of Nuclear Astrophysics,
3 October 2008
Volume 6, Issue 40 (33 Articles)
- # 5 - The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
- M. Pignatari (1,2), R. Gallino (3,4), G. Meynet (5), R. Hirschi (1,6), F. Herwig (1,7), M. Wiescher (2) ((1) Keele University, Keele, UK, (2) JINA, University of Notre Dame, Notre Dame, IN, USA, (3) Dipartimento di Fisica Generale, Universita' di Torino, Via Pietro Giuria 1, Torino, Italy, (4) Center for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria, Australia, (5) Geneva Observatory, Sauverny, Switzerland, (6) IPMU, University of Tokyo, Kashiwa, Japan, (7) Department of Physics & Astronomy, University of Victoria, Victoria, BC, Canada)
- arXiv.org - Astrophysics - Volume: 2008, Issue: 2 Oct
- arXiv:0810.0182 [ps, pdf, other]
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
